Add to ORKGObservations of recombination lines form normal H II regions, extended H II regions, nonthermal sources, and the H I medium are discussed. Detection of recombination lines from elements other than hydrogen may provide a means of identifying fossil Stromgren spheres at high temperature
A survey of the H272-alpha recombination line at 325 MHz has been made towards 53 directions in the ...
Aims. Observations of millimeter wavelength radio recombination lines (mm-RRLs) are used to search f...
We present constraints on the physical properties of the ionized gas responsible for hydrogen radio ...
Over the past forty years, investigations of radio recombination lines have become an effective way ...
We have made accurate calculations of recombination lines of H, He, C, and S from 100 GHz to 10 ?m (...
At the time of the last review of radio recombination line research in these pages (Dupree & Goldber...
Since their first detection 15 years ago, radio recombination lines from several elements have been ...
A survey of ten galactic HII regions provided the most extensive high frequency (near 8.6 GHz) recom...
Using the Very Large Array with an angular resolution of ~3", we have detected the hydrogen recombin...
Using the Very Large Array with an angular resolution of 3", we have detected the hydrogen recombina...
We present constraints on the physical properties of the ionized gas responsible for hydrogen radio ...
Using the Very Large Array (VLA) with an angular resolution of 3", we have detected the hydrogen rec...
Text no 1 Radio Recombination Lines (RRLs), discovered in the USSR in 1964, have become a powerful r...
Radio recombination lines are known to be observable at positions along the galactic ridge which are...
We report the detection of stimulated hydrogen radio recombination line (RRL) emission from ionized ...
A survey of the H272-alpha recombination line at 325 MHz has been made towards 53 directions in the ...
Aims. Observations of millimeter wavelength radio recombination lines (mm-RRLs) are used to search f...
We present constraints on the physical properties of the ionized gas responsible for hydrogen radio ...
Over the past forty years, investigations of radio recombination lines have become an effective way ...
We have made accurate calculations of recombination lines of H, He, C, and S from 100 GHz to 10 ?m (...
At the time of the last review of radio recombination line research in these pages (Dupree & Goldber...
Since their first detection 15 years ago, radio recombination lines from several elements have been ...
A survey of ten galactic HII regions provided the most extensive high frequency (near 8.6 GHz) recom...
Using the Very Large Array with an angular resolution of ~3", we have detected the hydrogen recombin...
Using the Very Large Array with an angular resolution of 3", we have detected the hydrogen recombina...
We present constraints on the physical properties of the ionized gas responsible for hydrogen radio ...
Using the Very Large Array (VLA) with an angular resolution of 3", we have detected the hydrogen rec...
Text no 1 Radio Recombination Lines (RRLs), discovered in the USSR in 1964, have become a powerful r...
Radio recombination lines are known to be observable at positions along the galactic ridge which are...
We report the detection of stimulated hydrogen radio recombination line (RRL) emission from ionized ...
A survey of the H272-alpha recombination line at 325 MHz has been made towards 53 directions in the ...
Aims. Observations of millimeter wavelength radio recombination lines (mm-RRLs) are used to search f...
We present constraints on the physical properties of the ionized gas responsible for hydrogen radio ...